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Article

The Zircon U-Pb Age, Hf Isotopes, and Lithogeochemistry of Ore-Bearing Rocks from the Archean Hongtoushan Volcanogenic Massive Sulfide Deposit in the North China Craton: Implications for Tectonic Setting

1
School of Resources and Civil Engineering, Northeastern University, Shenyang 110819, China
2
School of Resource & Materials, Northeastern University at Qinhuangdao, Qinhuangdao 066004, China
3
School of Earth and Space Sciences, Peking University, Beijing 100871, China
*
Author to whom correspondence should be addressed.
Submission received: 25 January 2024 / Revised: 14 March 2024 / Accepted: 24 March 2024 / Published: 29 March 2024
(This article belongs to the Special Issue Mineral Resources in North China Craton)

Abstract

:
Volcanogenic massive sulfide (VMS) deposits are globally significant sources of metals. The Hongtoushan VMS deposit is the only large Archean Cu-Zn VMS deposit in the North China Craton, carrying substantial economic value. Significant deformation and metamorphism have made the tectonic setting of the Hongtoushan VMS deposit the subject of extensive debate. This study investigates the petrogenesis and chronology of the ore-bearing host rocks from the Hongtoushan Cu-Zn VMS deposit in the North China Craton. By utilizing whole-rock geochemical analyses and zircon dating, this research sheds light on the origin and evolution of the ore-bearing rocks within the deposit. The whole-rock geochemical analysis data indicate that the Hongtoushan ore-bearing rock series is mainly composed of amphibole plagioclase gneiss (basalt protolith) and biotite plagioclase gneiss (andesite and rhyolite protolith), suggesting a complete volcanic cycle from basic to medium-acidic volcanic rocks. The amphibole plagioclase gneiss has slight LREE enrichment patterns with unremarkable depletions of Nb, Ta, and Ti and belongs to contaminated ocean plateau basalt (OPB) in terms of composition, which is generally interpreted as being generated from the mantle plume head. Meanwhile, the biotite plagioclase gneiss has relatively steep LREE enrichment distribution patterns with remarkable negative Ta, Nb, and Ti anomalies and a wide range of Zr/Y ratios, indicating their classification as FI- and FII-type felsic rocks; they were likely formed through the fractional crystallization of basic magma combined with crustal assimilation. When combined with the zircon dating results, the ore-bearing host rocks of the Hongtoushan VMS deposit were generated via a continuous magmatic evolution process. The zircon dating of the host rocks indicates a formation age of between 2609 and 2503 Ma, with metamorphic events between 2540 and 2466 Ma, which is consistent with the 2.5 Ga-related global mantle plume event. Further research shows that the ore-bearing host rocks are more likely to have been formed in a mantle plume-related stretching environment, possibly a margin rift.

1. Introduction

The Qingyuan granitic-greenstone belt (QGB) was the first identified Archean greenstone belt in China. Numerous Cu-Zn deposits of varying sizes have been discovered in the QGB, serving as significant sources of copper, zinc, and lead in China. As the largest volcanogenic massive sulfide (VMS) deposit in the QGB, the Hongtoushan VMS deposit has been exploited until now. The Hongtoushan Cu-Zn deposit has been the focus of much research due to its unique metallogenic environment and model. Significant geological and geochemical research has been conducted on the Hongtoushan VMS deposit since its discovery in 1957 [1,2], resulting in its classification as a VMS-type deposit and its designation as the “Hongtoushan type” by Chinese geologists [3].
The ancient Archean Hongtoushan VMS deposit has experienced significant deformation and metamorphism, leading to the development of ore bodies with intricate and complex geometries [4,5]. The tectonic setting of the Hongtoushan VMS deposit has been the subject of extensive debate. Previous scholars have proposed multiple hypotheses, which can be broadly categorized into two main schools of thought: the magmatic arc model and the mantle plume model. However, these two schools of thought are somewhat inconsistent with each other and have failed to explain certain factors based on field geological and geochemical data.
Supporters of the mantle plume model, such as Franklin et al. (2005) [6], argue that VMS mineralization universally requires a submarine heat source in an extensional tectonic setting, including oceanic environments or marine basins developed on rifted crusts. Zhai et al. (1985) [1] proposed that the supracrustal volcanic rocks (greenstone belt) erupted in a paleo-continental rift above a hotspot (mantle plume), whereas Wu et al. (2013) [7] suggested that the terrain was formed above a mantle plume based on lithological characteristics and anti-clockwise pressure–temperature paths involving a period of isobaric cooling. However, these theories face a compelling question in terms of explaining the magmatic arc characteristics of the host rocks in the Hongtoushan deposit. On the other hand, proponents of the magmatic arc model, such as Li et al. (2000) and Wan et al. (2005) [8,9], argue that the QGB evolved in a continental arc environment followed by arc collision. However, in the eastern North China Craton (NCC), Neoarchean magmatism extends over a width of more than 800 km [10], and the prominent structural feature is the dome-and-keel structure [11], which is inconsistent with subduction processes.
In order to shed light on the origin and tectonic setting of the Hongtoushan VMS deposit, this study investigates the petrogenesis and zircon chronology of the ore-bearing host rocks from the Hongtoushan Cu-Zn VMS deposit in the North China Craton, contributing to the understanding of the geological processes involved in the formation of Hongtoushan VMS deposits and tectonic evolution in the Archean period.

2. Local Geology

2.1. Regional Geology

The Hongtoushan Cu-Zn VMS deposit is situated within the Qingyuan granite-greenstone belt, which forms a part of the North China Craton (NCC) (Figure 1A). The NCC encompasses an Archean to Paleoproterozoic metamorphic basement overlayed by Mesoproterozoic to Cenozoic unmetamorphosed cover. The metamorphic basement rocks exhibit ages ranging from 3.8 to 3.2 Ga [9,12,13]. Neoarchean metamorphic rocks are predominantly composed of 2.6–2.5 Ga tonalite–trondhjemite–granodiorite (TTG) gneisses, ~2.5 Ga syntectonic granites and various supracrustal rocks that experienced greenschist to granulite facies in regional metamorphism and polyphase deformation around 2.5 Ga [14,15,16]. The NCC is divided into two major Archean to Paleoproterozoic blocks, the eastern and western blocks, separated by the Paleoproterozoic Trans-North China orogenic belt [17]. The Qingyuan greenstone belt is located at the northern margin of the eastern block and, together with large volumes of granitoid compositions, it is commonly known as the Qingyuan Group [9,18] (Figure 1B). The Qingyuan Group is divided into the Hunbei and Hunnan terranes by the Hunhe fault [19,20]. The greenstone in the Hunbei terrane comprises a sequence of gneiss and amphibolite that is further classified into the Shipengzi, Hongtoushan, and Nantianmen formations, which experienced amphibolite to granulite facies metamorphism between 2.9 and 2.8 Ga [1,19]. The VMS deposit is the predominant mineral resource in the Qingyuan greenstone belt, wherein the Hongtoushan VMS deposit stands out as the largest in the region. The size and location of Cu-Zn mineralization in the area are controlled by impermeable volcanic layers [21].

2.2. Ore Deposit Geology

The Hongtoushan VMS deposit is a significant Archean VMS Cu-Zn deposit located in the Hunbei district. Local residents began the surface mining of the deposit in the early 1930s, and large-scale underground operations started in the 1960s following systematic drilling. The deposit has a metal reserve of 0.5 Mt Cu at 1.5% to 1.8% Cu, 0.7 Mt Zn at 2.0% to 2.5% Zn, 20 t Au at 0.5 to 0.8 g/t Au, and 1000 t Ag at 20 to 60 g/t Ag, respectively [2]. Mining operations have reached a depth of 1337 m [23].
The primary ore deposits in the area are confined within the “rhythmic member” of the upper section of the Hongtoushan formation, which is mainly composed of biotite plagioclase gneiss and hornblende plagioclase gneiss and can be divided into seven layers. From top to bottom, these layers include (1) a 12 m-thick layer of biotite gneiss and quartz-feldspar gneiss with intercalations of plagioclase hornblende gneiss; (2) a 25 m-thick layer of garnet quartz plagioclase gneiss intercalated with granulite; (3) a 20 m-thick layer of plagioclase amphibole gneiss and biotite plagioclase gneiss intercalations; (4) a 20 m-thick layer of plagioclase hornblende gneiss intercalated with thin biotite plagioclase gneiss; (5) a 20 m-thick layer of biotite plagioclase gneiss with plagioclase hornblende gneiss; and (6) a 10 m-thick layer of plagioclase hornblende gneiss, biotite plagioclase gneiss, and interbedded plagioclase hornblende gneiss (Figure 2G). Petrological and geochemical investigations indicate that the protolith of meta-volcanic rocks in the Jinfengling and Hongtoushan formations is tholeiite to calc-alkalic volcanic rocks [1,4].
The massive sulfide ores in the area are hosted by rocks that have undergone upper amphibolite facies metamorphism [24]. The surrounding rocks are mainly composed of amphibolite gneiss, sillimanite-biotite gneiss, and biotite plagioclase gneiss, and the protoliths are believed to be continuously differentiated volcanic rocks varying in composition from basic to intermediate acid volcanic rocks [5] (Figure 2G).
The Archean Qingyuan greenstone belt has undergone multiple episodes of deformation, metamorphism, intrusion by granites, and migmatization, resulting in the Hongtoushan VMS deposit having a highly intricate structure. Above a depth of −467 m, the ore bodies display a Y-shaped structure, where the two branches extend towards the east. As they progress, these two branches combine and form a unified entity towards the west (Figure 3A,C). According to previous research results [22,23], three periods of tectonic deformation have been identified in the Hongtoushan VMS deposit. In the initial phase, the north–south tight fold was generated in response to the east–west extrusion force. Following this, the north–south extrusion force led to the formation of the east–west plunging vertical fold in the subsequent stage. Under tectonic compression, the original ore body migrated from the limbs towards the hinge zone, resulting in the thickening and upgrading of the ore body and the formation of the “ore pillar” (Figure 3B). Lastly, driven by east–west extrusion and north–south torsion, the third stage culminated in the development of the north–south open fold. Fold deformation transforms the occurring forms of the ore body and plays an ore-controlling and ore-hosting role in the transformation.
The deposit can be classified into two types of ores: massive and disseminated ore. The dominant ore minerals are pyrite, pyrrhotite, sphalerite, and chalcopyrite, with minor amounts of magnetite, galena, molybdenite, argentite, and electrum. The gangue minerals mainly consist of quartz, plagioclase, biotite, phlogopite, sericite, garnet, gahnite, sillimanite, and other minerals. The wall rock alteration is characterized by tremolitation, phlogopitization, sericitization, silicification, chloritization, and carbonation (Figure 4).

3. Samples and Analytical Methods

3.1. Sample Descriptions

The samples were collected from ore-bearing metamorphic rocks (the rhythmic member) (Figure 2A–F) and classified into two major categories according to mineral composition: amphibole plagioclase gneiss and biotite plagioclase gneiss. For these two groups of rocks, we proceeded to conduct a comprehensive suite of analyses. In total, 20 rock samples were selected for major and trace (rare earth) element analyses, while subsequent preliminary microscopic observations confirmed the presence of a sufficient number of zircon grains. Six rock samples (including three amphibole plagioclase gneiss and three biotite plagioclase gneiss samples) were finally chosen for zircon U-Pb dating and a Hf isotope analysis.

3.2. Analytical Methods

3.2.1. Whole-Rock Geochemistry Analysis

Whole-rock major and trace (rare earth) element analyses were performed at the Geoanalytical Center of Nuclear Industry in Beijing using X-ray fluorescence (XRF) spectrometry and inductively coupled plasma mass spectrometry (ICP-MS), respectively. The analytical uncertainties for major elements are 1%~3%, and this is based on the GB/T14506.28-2010 standard [26]. For trace element and rare earth element analyses, in accordance with the DZ/T0223-2001 standard [27], rock powders (50 mg) were dissolved using mixed acids (HF + HClO   4 ) in capped Savillex Teflon beakers at 120 °C for 6 days and were subsequently dried to wet salt and then re-dissolved in 0.5 mL HClO   4 . The solutions were then evaporated to wet salt at 140 °C and re-dissolved in 1 mL HNO   3 and 3 mL water for 24 h at 120 °C. The solutions were diluted in 2% HNO   3 for analysis. The uncertainties based on the replicate analyses of internal standards are ±5% for REE and ±5%~10% for trace elements.

3.2.2. Zircon CL Images and U-Pb Dating

Zircon grains were isolated from whole-rock samples through a magnetic and heavy liquid separation technique at Beijing GeoAnalysis Co., Ltd., Beijing, China. These zircon grains were subsequently randomly embedded in epoxy mounts, and then the mounts were polished for sectioning. Detailed documentation of all zircon grains was carried out using transmitted and reflected light micrographs, along with cathodoluminescence (CL) images, to elucidate their internal structures. The CL images of the zircon grains were captured at Beijing GeoAnalysis Co., Ltd. by utilizing a JEOL IT-500 SEM equipped with a Delmic CL system.
Zircon U-Pb dating was performed using a Resolution SE-type 193 nm deep-ultraviolet laser ablation sampling system (Applied Spectra, Fremont, CA, USA) and an S155-type double-volume sample cell at Beijing GeoAnalysis Co., Ltd. A fixed 30 μ m diameter laser beam was utilized with a laser pulse frequency of 6 Hz and a fluence of 5 J/cm   2 . Zircon GJ-1 (599.8 ± 4.5 Ma; Jackson et al., 2004 [28]) and 91,500 (1062.4 ± 0.4 Ma; Wiedenbeck et al., 1995 [29]) served as primary and secondary reference materials, respectively. Typically, 20 s of a gas blank and 35–40 s of the signal interval were collected for data processing. Deep fractionation correction was carried out based on an exponential equation (Paton et al., 2010 [30]). NIST 610 was employed to calibrate the trace element content. The measured ages of the reference materials in the batch were as follows: 91,500 (1061.5 ± 4.1 Ma, 2 δ , MSWD = 0.55, n = 32), GJ-1 (600.5 ± 2.9 Ma, 2 δ , MSWD = 0.95, n = 32), showing consistency with the reference values within a specific uncertainty range. The zircon Plesovice was dated as ‘‘unknown samples” and yielded a weighted mean   206 Pb/   238 U age of 336.1 ± 1.1 Ma (2 δ , MSWD = 0.43, n = 32), aligning closely with the reference value within a defined uncertainty (337.13 ± 0.37 Ma; Sláma et al., 2008 [31]). The analysis results were processed using ICPMSDataCal 10.9 software (Liu et al., 2010 [32]). The concordia plots and weighted average U-Pb ages were determined using the IsoplotR 3.3 online program [33].

3.2.3. Zircon Hf Isotope Analysis

An in situ zircon Hf isotope analysis was conducted utilizing a RESOlution SE 193 laser ablation system coupled with a Thermo Fisher Scientific Neptune Plus MC-ICP-MS at Beijing Createch Testing Technology Co., Ltd., Beijing, China. The instrumental parameters and data acquisition methodologies were detailed by Hou et al. (2009) [34]. A stationary spot with a beam diameter of approximately 55 μ m was employed. Helium served as the carrier gas to transport the ablated sample aerosol, mixed with argon from the laser ablation cell, to the MC-ICP-MS torch through a mixing chamber. The   176 Lu/   175 Lu = 0.02658 and   176 Yb/   173 Yb = 0.796218 ratios were determined to correct for the isobaric interferences of   176 Lu and   176 Yb on   176 Hf. For instrumental mass bias correction, the Yb isotope ratios were normalized to   172 Yb/   173 Yb = 1.35274 and the Hf isotope ratios to   179 Hf/   177 Hf = 0.7325 using an exponential law. It was assumed that the mass bias behavior of Lu followed that of Yb. The mass bias correction protocol was outlined by Hou et al. (2009) [34]. The zircon international standard GJ-1 was utilized as the reference standard. The measured   176 Hf/   177 Hf ratios of the standard zircon GJ-1 were 0.282001 ± 33 (2 δ , n = 37), which closely resembled the recommended   176 Hf/   177 Hf ratio of 0.282003 ± 18 [35].

4. Results of Zircon Isotope Dating

The zircons separated from two types of gneiss in the ore-bearing wall rocks of the Hongtoushan “rhythmic member” exhibit three major groups in CL images. However, due to complex deformation and metamorphism, we will also utilize the contents of U and Th, as well as the Th/U ratio, to collectively constrain the genesis of the zircons. One main group of zircons is prismatic or fragmented crystals with length/width ratios of 3:1 to 5:1; these display relatively blurred oscillatory or sector zones. The second group of zircons have short prismatic or nearly rounded crystals with length/width ratios of 1:1 to 1.5:1, and the third group of zircons have different widths of core–rim structures that are characterized by clear oscillatory zoned cores surrounded by dark rims. Some grains even have clear corrosion rims. The analyzed data of the Hf isotopic and U-Pb dating are listed in Table A1. Detailed descriptions will be provided for each sample of the two types of gneiss.

4.1. Amphibole Plagioclase Gneiss

4.1.1. Sample HTS-1605-2

The zircon grains extracted from sample HTS-1605-2 are characterized by prismatic crystals with length-to-width ratios ranging from 3:1 to 5:1. In the CL images, the zircons are gray in color, and most of them exhibit blurred oscillatory zoning with a wide range of Th and U content (Th = 17.00–267.00 ppm; U = 80.30–373.00 ppm) and higher Th/U ratios, ranging from 0.11 to 1.08 (Figure 5A,B). This part of the zircons shows affinity with a magmatic origin [36]. A total of 15 U-Pb dating analyses were performed on this part of the zircons; the samples yielded a concordant age of 2510.5 ± 3.9 Ma (N = 17; MSWD = 2.1), which is consistent with the weighted mean age of 2512.1 ± 3.9 Ma (N = 17/17; MSWD = 3.4; see Figure 5C). At the same time, another few zircons display gray cores with a light, narrow corrosion field and unstructured dark rims in the CL images. Three analyses of the rims were performed; they exhibit low Th/U ratios ranging from 0.02 to 0.09 (Th = 3.66–26.80 ppm; U = 97–197 ppm) (Figure 5A,B), and have a   207 Pb/   206 Pb mean age of 2472 ± 20 Ma. We consider that the rocks erupted at 2510.5 ± 3.9 Ma and were modified by a metamorphic event at 2472 ± 20 Ma.

4.1.2. Sample HTS-1605-6

Most zircons found in sample HTS-1605-6 are characterized by prismatic or fragmented crystals with length-to-width ratios ranging from 1:1 to 3:1. They are gray in color, exhibit blurred oscillatory or sector zoning in the CL images and have relatively higher contents and concentrated ranges of Th and U (Th = 76.78–219.04 ppm; U = 261.33–1118.18 ppm). The Th/U ratios range from 0.115 to 0.542 (see Figure 6A,B). These zircon signatures indicate a magmatic origin [36]. A total of 13 U-Pb datings were conducted on sample HTS-1605-6, and these yielded an upper intercept age of 2528.8 ± 6.4 Ma (N = 13; MSWD = 0.56). The age is consistent with a weighted mean age of 2514.4 ± 4.0 Ma (N = 13; MSWD = 2.6), which is indicative of the formation age (see Figure 6C).

4.1.3. Sample HTS-1605-9

Similar to sample HTS-1605-2, most of the zircon grains in sample HTS-1605-9 exhibit prismatic crystals with length-to-width ratios of 2:1 to 5:1. Most of the zircons display core–rim structures, with a wide range in content regarding Th and U (Th = 11.30–978.00 ppm; U = 36.10–1039.00 ppm); they have Th/U ratios ranging from 0.123 to 0.941. A total of 15 points yield an upper intercept age of 2593 ± 11Ma (N = 15; MSWD = 2.5, see Figure 7C), which can be considered as the formation age of HTS-1605-2. In contrast, few of them have relatively gray cores with blurred, irregular banded zoning rims in the CL images and have lower Th and U contents (Th = 6.35–26.00 ppm; U = 125.40–430.00 ppm), with Th/U ratios that are conspicuously lower than the ratios in the cores, ranging from 0.044 to 0.066 (see Figure 7A,B). These zircon signatures indicate the recrystallization of metamorphism. A total of four analyzed samples were obtained from the zircon rims. They have a   207 Pb/   206 Pb age range from 2529 ± 23 to 2497 ± 23 Ma and yield an upper intercept age of 2526 ± 13 Ma (N = 4; MSWD = 0.19), which can be considered the metasomatism age.

4.2. Biotite Plagioclase Gneiss

4.2.1. Sample HTS-1605-1

The zircons extracted from sample HTS-1605-1 display prismatic crystals with length-to-width ratios of 1:1.5 to 1:3. The zircon grains are round in shape with blurred sector zoning and most have extremely low contents and concentrated ranges of Th and U (Th = 7.60–26.00 ppm; U = 421.00–2060.00 ppm), and the Th/U ratios range from 0.012 to 0.040, which are indicative of their metamorphic origin (see Figure 8A,B). A total of 19 U-Pb dating analyses were performed on the zircon grains, and 16 points with low Th/U ratios yielded an upper intercept age of 2471.8 ± 2.6 Ma (N = 16; MSWD = 0.81) and corresponded to a weighted mean age of 2471.2 ± 2.0 Ma (N = 16; MSWD = 4.7), which is indicative of the recrystallization age (Figure 8C). Some individual zircons exhibit a core–rim structure, with a bright, small, and circular core surrounded by a darker rim. Due to the small size of the cores, we only tested three zircons. Their cores have higher Th/U ratios ranging from 0.216 to 0.438, indicating that the cores are of magmatic origin. Three core points have a   207 Pb/   206 Pb age range of 2481 ± 23 to 2466 ± 21 Ma.

4.2.2. Sample HTS-1605-3

The zircons obtained from sample HTS-1605-3 display prismatic crystals with length-to-width ratios of 1:1.5 to 1:3. The zircon grains generally display relatively bright cores and dark rims. Most of the zircon grains are small in size, with extremely low Th/U ratios ranging from 0.005 to 0.057 (Th = 2.28–48.23 ppm; U = 391.94–1200.00 ppm). After comparing the Th/U ratios between the cores and rims, combined with the uniformly positive ε Hf(t) and relatively concentrated ages, we consider that the zircon grains in HTS-1605-3 are more likely to be inherited zircons, and the low Th/U ratios could be attributed to the influence of late-stage hydrothermal fluids [37] (see Figure 9A,B). A total of 15 analyses yielded an upper intercept age of 2509.0 ± 5.8 Ma (N = 15; MSWD = 0.25), which is consistent with the weighted mean age of 2503.3 ± 2.8 Ma (N = 15; MSWD = 0.91) (see Figure 9C). The results approximately represent the formation age of biotite plagioclase gneiss.

4.2.3. Sample HTS-1605-8

Most zircons obtained from sample HTS-1605-8 are mostly irregular crystals with length-to-width ratios of approximately 1:1.5 to 2:1, appearing light gray in the CL images, with faint zoning patterns observed internally. A few zircons have small, bright residual cores. These characteristics indicate that they were more likely formed by recrystallization (Figure 10A). However, due to the small size of the residual cores, they were not suitable for testing. Therefore, all the tests were conducted on homogeneous zircon grains. They have Th and U contents of Th = 21.20–333.20 ppm and U = 56.00–844.00 ppm and Th/U ratios ranging from 0.108 to 1.169. A total of 28 U-Pb dating analyses yielded a concordia age of 2468.5 ± 2.4 Ma (N = 28; MSWD = 1.2), and this correspond with the mean age of 2469.0 ± 2.4 Ma (N = 28/28; MSWD = 1.5), which may indicate the recrystallization age of the zircons (Figure 10C).

5. Results of Hf Isotopic Analysis

The Lu-Hf data on the zircons from the individual samples are briefly listed in Table 1. A total of 40 of the Lu-Hf isotopes analyzed were obtained from the zircon grains from amphibole plagioclase gneiss. The results are presented in Table A2. The results of the amphibole plagioclase gneiss samples show the initial   176 Hf/   177 Hf ratios range from 0.28128 to 0.28144. The ε Hf(t) values are in the range of 3.91 to 10.45. The TDM1 ages are between 2687.69 Ma and 2453.51 Ma, and the TDM2 ages range from 2776.75 to 2411.13 Ma. Meanwhile, 48 Lu-Hf isotope analyses were performed on the zircon grains from biotite plagioclase gneiss. The results of biotite plagioclase gneiss samples show the initial   176 Hf/   177 Hf ratios range from 0.28126 to 0.28143. The ε Hf(t) values are in the range of 3.07 to 9.16. The TDM1 ages are between 2728.02 Ma and 2489.84 Ma, and the TDM2 ages range from 2838.15 to 2469.98 Ma.

6. Geochemical Result of Ore-Bearing Metamorphic Rocks

6.1. Assessing Element Mobility

The Archean Hongtoushan VMS deposit has undergone amphibolite-to-granulite facies metamorphism and multi-period tectonic deformation [22]; it is necessary to evaluate the impact of high-grade metamorphism on element mobility, which may alter the geochemical properties of host rocks.
Altered samples generally have an LOI (enrichment in loss on ignition) of >6 wt% or δ Ce < 0.9 or >1.1 [38]. Moreover, the “alteration box plot” (Figure 11) from Large et al. (2001) [39] is also used to assess element mobility. In the CCPI versus AI diagram, the samples plotted in the least altered box are considered unaffected by hydrothermal alteration. After removing the obviously altered samples, 20 samples were identified for further discussion (Table A3). Previous studies have demonstrated that Zr is one of the most stable elements [38,40] and is appropriate for assessing element mobility. By comparing Zr diagrams with other select elements, good correlations among Zr and HFSEs and transition elements are observed (Figure 12I–L). These elements will be further discussed in terms of petrogenesis, magma signatures, and tectonic settings.

6.2. Major Element Composition

The major element composition of the ore-bearing metamorphic rocks is summarized in Table A3. The results show that the ore-bearing metamorphic rocks have a continuous oxide content. The biotite plagioclase gneiss samples have the following chemical compositions: SiO   2 ranging from 64.64 to 84.42 wt%, Fe   2 O   3 T ranging from 1.64 to 7.67 wt%, TiO   2 ranging from 0.10 to 0.61 wt%, MgO ranging from 0.33 to 4.79 wt%, K   2 O ranging from 0.74 to 3.59 wt%, CaO ranging from 0.77 to 4.84 wt%, Al   2 O   3 ranging from 6.94 to 16.46 wt%, and Na   2 O ranging from 1.93 to 5.85 wt% (see Table 2). In comparison, the amphibole plagioclase gneiss has lower values: SiO   2 ranging from 47.63 to 56.53 wt%, Fe   2 O   3 T ranging from 8.75 to 13.21 wt%, TiO   2 ranging from 0.52 to 2.44 wt%, MgO ranging from 3.17 to 7.42 wt%, K   2 O ranging from 0.34 to 2.97 wt%, and CaO ranging from 3.02 to 11.57 wt%, but it has a higher Na   2 O content, ranging from 2.27 to 3.71 wt%, and Al   2 O   3 content, ranging from 14.25 to 16.67 wt% (see Table 2). There is obviously a negative correlation between the content of selected oxides and the content of SiO   2 , except for the contents of Na   2 O and K   2 O (Figure 12A–H).

6.3. Trace and Rare Earth Elements

Based on the data from the ore-bearing host rocks from the Hongtoushan VMS deposit, transition metal elements, such as Co (27.80–47.70 ppm; avg: 34.42 ppm), Ni (34.10–131.50 ppm; avg: 65.82 ppm), Cu (10.90–67.10 ppm; avg: 37.65 ppm), and Zn (77.00–366.00 ppm; avg: 171.50 ppm), are relatively slightly more concentrated in amphibole plagioclase gneiss than in biotite plagioclase gneiss, which exhibits Co, Ni, Cu, and Zn concentrations of 2.60–19.90 ppm (avg: 8.49 ppm), 2.10–131.50 ppm (avg: 23.89 ppm), 2.90–80.40 ppm (avg: 21.36 ppm), and 22.00–585.00 ppm (avg: 103.43 ppm), respectively. On the other hand, the biotite plagioclase gneiss is relatively enriched in LILEs (large-ion lithophile elements): (K: 6142.96–29,801.67 ppm, avg: 15,351.48 ppm; Rb: 14.1–109.25 ppm, avg: 51.28 ppm; Sr 47.30–723.00 ppm, avg: 306.61 ppm; Ba 78.70–2810.00 ppm, avg: 5878.39 ppm).
In the chondrite-normalized REE pattern diagram for the amphibole plagioclase gneiss, the samples display near flat to weakly LREE-enriched REE patterns, with a mean La/Yb   N value of 3.91, and weakly negative δ Eu anomalies, with a mean δ Eu value of 0.84 (Figure 13B). In the primitive mantle-normalized spider diagram for the amphibole plagioclase gneiss, the samples exhibit weak negative anomalies in Ta, Nb, and Ti and very weak to medium negative Zr-Hf anomalies (Figure 13A). In contrast, the biotite plagioclase gneiss in the chondrite-normalized REE pattern diagram exhibits remarkable LREE-enriched patterns, with a wide range of La/Yb   N from 3.25 to 60.68, and they have a δ Eu value range from 0.39 to 2.53 (Figure 13D). In the spider diagram, the samples show more prominent negative Ta, Nb, Ti, and P anomalies and positive Zr-Hf anomalies (Figure 13C). Notably, no Ce anomalies are observed in any of the host rocks, with mean δ Ce values of 1.00 and 0.96 for amphibole plagioclase gneiss and biotite plagioclase gneiss, respectively (see Table 2).

7. Discussion

7.1. Petrogenesis of Hongtoushan Ore-Bearing Rocks

Ga versus Zr/TiO   2 and Nb/Y versus TiO   2 diagrams are used to classify metamorphic rocks in the Hongtoushan VMS deposit. In the Ga versus Zr/TiO   2 diagram, the amphibole plagioclase gneiss samples are mostly plotted in the basalt field, while the biotite plagioclase gneiss samples are plotted in the andesite to rhyolite field (Figure 14A). In the Nb/Y versus Zr/TiO   2 diagram, the amphibole plagioclase gneiss samples are mostly plotted in the basalt and andesite/basalt field, while the biotite plagioclase gneiss samples are placed in the andesite, rhyodacite, rhyolite, and trachyandesite field (Figure 14B). Meanwhile, the compositions of metamorphic rocks show a continuous variation trend for the major element versus SiO   2 diagrams (Figure 12). According to this study, and when combined with previous research [22], the amphibole plagioclase gneiss has a protolith of basalt, while the biotite plagioclase gneiss has protoliths of andesite and rhyolite. It is believed that the studied area has experienced a complete volcanic cycle from basic volcanic rocks to medium-acidic volcanic rocks.

7.1.1. Crustal Contamination and Fractional Crystallization

It is essential to note that the composition of any given magma can be influenced by various factors, such as the mantle source’s composition, melting degree, fractionation, and, especially, crustal contamination. The magma can become enriched in elements such as Zr, Hf, and LREEs while being depleted in Nb and Ta under significant crustal contamination [43,44,45,46,47,48,49,50,51]. This may result in a signature depleted in Nb, Ta, and Ti, similar to that observed in subduction-related magmatism, which is referred to as a “fake subduction signal” by Ernst (2005) [52]. Thus, it is imperative to conduct a more comprehensive assessment of the potential factors that could potentially exert an influence on the constituent composition of the magma.
Previous protolith recovery results indicate that the protolith of amphibole plagioclase gneiss is a series of basalt. However, the amphibole plagioclase gneiss of the Hongtoushan VMS deposit displays weakly enriched LREE patterns with weakly negative Nb, Ta, and Ti anomalies and insignificant- to medium-negative Zr and Hf anomalies (Figure 13A,B). In the Th/Yb versus Nb/Yb diagram (Figure 15A), the amphibole plagioclase gneiss samples are concentrated around E-MORB and SCLM end-members within the mantle array (the field between the dashed lines) and show a remarkable trend to the vector of fractional crystallization and an insignificant trend of crustal contamination. In the Th/Nb versus La/Sm diagram (Figure 15B), all samples except one have extremely high Th/Nb ratios, which may have been significantly affected by crustal contamination. The rest of the samples are mainly plotted near the primitive area and display a weak trend toward upper-crust fractional crystallization. Therefore, it can be presumed that the amphibole plagioclase gneiss suffered limited crustal contamination.

7.1.2. Amphibole Plagioclase Gneiss

The previous results suggest that the amphibole plagioclase gneiss has undergone slight crustal contamination. Thus, the weak enrichment of LREE patterns and weak negative Nb, Ta, and Ti anomalies are unlikely to have been caused by crustal contamination completely. These characteristics are more likely inherited from enriched mantle sources. In the Nb/Yb versus Th/Yb diagram, the amphibole plagioclase gneiss is mainly plotted in the field near the E-MORB end-member and shows a trend that is parallel with MORB-OIB, reflecting the mantle plume source [55]. The samples slightly falling above the array can be interpreted by the limited crustal contamination mentioned above (Figure 16A). Likewise, in the Nb/Y versus Zr/Y diagram, the amphibole plagioclase gneiss is mainly plotted near the end-member of primitive mantle within the field of OPB (ocean plateau basalt) and displays a similar vector to the batch melting array (Figure 16B). This type of mantle melting means that the melt is in equilibrium with the mantle residue until it separates from it (segregates) and intrudes into the crust [57,58]. Therefore, based on the analytical results, we propose that amphibole plagioclase gneiss is more likely generated from the mantle plume head.

7.1.3. Biotite Plagioclase Gneiss

Based on the REE patterns, Eu anomalies, Zr/Y ratios, and trace element abundances, Hart et al. (2004) [59] categorized felsic rocks in Archean terranes into four groups: FI to FIV. The FI group exhibits high Zr/Y ratios, low HFSE abundances, relatively steep REE patterns, and Eu anomalies ranging from weakly negative to moderately positive. In contrast, the FIII rhyolites may be subdivided into two types. FIIIa rhyolites exhibit variable negative Eu anomalies, low Zr/Y, and intermediate abundances of HFS elements. FIIIb rhyolites exhibit pronounced negative Eu anomalies, low Zr/Y, and high abundances of HFSEs. The FIV group contains rhyolites and high-silica rhyolites, which are characterized by flat to slightly LREE-depleted REE patterns and low REE and HFSE abundances. The biotite plagioclase gneiss of the Hongtoushan VMS deposit displays significant enrichment in LREEs (avg: (La/Yb)   N = 18.22) and remarkable negative Ta, Nb, and Ti anomalies with relatively high Zr/Y ratios (3.64–75.59) (Figure 13C,D). In the (La/Yb)   N versus Yb   N diagram (Figure 17A), the biotite plagioclase gneiss of the Hongtoushan VMS deposit predominantly shows an affinity with FI-type and FII-type felsic volcanic rocks.
FII group rocks are generally considered to host few deposits. Researchers proposed that these rocks are generally interpreted as the products of lower-temperature melts (<900 °C) at deeper levels in the crust (>10 km). Due to the lower temperature and loss of heat during transport to the surface, they have less potential to drive the hydrothermal convection system for a long time [60,61]. However, Cathles et al. (1997) [62] and Barrie et al. (1999) [63] claim that the heat engines that drive ore forming should not be solely considered. Thermal models showed that the period of time that an intrusion is able to sustain high-temperature hydrothermal convection is primarily a function of the mass of the intrusion, the temperature of the magma, and the temperature and permeability of the host rocks. Larger, higher temperature mafics or ultramafic intrusions emplaced at deeper crustal levels (10–18 km), where the country rocks are characterized by a lower permeability and higher rock-wall temperatures, favor the generation of long-lived, high-temperature, convective hydrothermal systems (e.g., Cathles et al. (1997) [62]).
Figure 17. (A) (La/Yb)   N versus Yb   N diagram from Hart et al. (2004) [59]; (B) Zr/Y versus Zr diagram of the Hongtoushan VMS deposit (from Liu (2018) [64] and Rollinson, H. (1993) [65]).
Figure 17. (A) (La/Yb)   N versus Yb   N diagram from Hart et al. (2004) [59]; (B) Zr/Y versus Zr diagram of the Hongtoushan VMS deposit (from Liu (2018) [64] and Rollinson, H. (1993) [65]).
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In the previous discussion, we discovered that the parent magma of the amphibole plagioclase gneiss is formed by the partial melting of about 10%–30% garnet-spinel lherzolite. The tectonic setting is interpreted as a margin rift associated with mantle plume activity. A continuous magmatic evolution trend is shown by gradual changes in the basaltic to rhyolitic composition of the original volcanics (Figure 12 and Figure 14A) and the stable fractional crystallization trend with limited crustal assimilation trends in the Zr/Y versus Zr diagram, which displays a commonly continuous magmatic evolution process. Therefore, the petrogenesis of biotite plagioclase gneiss can be more reasonably interpreted as crustal assimilation combined with the fractional crystallization of basic magma (the magma source of amphibole plagioclase gneiss) in the rift environment. The stretching environment provided by rift structures and the high-temperature heat source from the mantle plume activity create ideal conditions for long-term hydrothermal reactions and heat conduits, contributing to the formation of large VMS deposits [59].

7.2. Chronology and Tectonic Implications of the Hongtoushan Deposit

The Hongtoushan Cu-Zn deposit is a typical VMS deposit and has undergone multiple deformation and metamorphic events since its formation. The ore bodies that form the deposit are generally stratified and controlled by the rhythmic member host rocks in the Hongtoushan formation [22]. This indicates that the formation age of the host rocks should be consistent with the formation age of the VMS deposit. The age determination of the ore-bearing host rocks is of great significance for constraining the formation time of the Hongtoushan VMS deposit. However, multiple episodes of high-grade metamorphism and deformation make isotopic age determination complex. Zircon has a very high Hf content and relatively low Hf diffusion, and the Hf isotope ratios are significantly insensitive to high-grade deformation and alteration [66]. By combining this with the results of the zircon U-Pb dating and Hf isotopes, as well as the geochemistry of the ore-bearing host rocks, we aimed to determine the chronology of the Hongtoushan VMS deposit.
Based on the results, the zircons in the amphibole plagioclase gneiss sample are concentrated around the age of ~2.5 Ga. The zircons have clear microscopic characteristics of magmatic origin, with a narrow and concentrated Th/U content ratio. Thus, the age of 2593 ± 11~2510.5 ± 3.9 Ma can approximately represent the formation age of amphibole plagioclase gneiss, and 2526 ± 13~2472 ± 20 Ma can approximately represent the metamorphic age of amphibole plagioclase gneiss. In biotite plagioclase gneiss, most zircons have already undergone metamorphism, and some retain inherited cores, showing a consistent metamorphic age of 2471.8 ± 2.6~2468.5 ± 2.4 Ma. When comparing the younger ages of the amphibolite plagioclase gneiss (2510.5 ± 3.9 Ma in sample HTS-1605-6) with the core points of the biotite plagioclase gneiss (2509.0 ± 5.8 Ma for HTS-1605-3), it can be reasonably interpreted that the zircon cores in the biotite plagioclase gneiss are more likely inherited from the grains of the amphibolite plagioclase gneiss. Collectively, a compilation of the available zircon geochronology results reveals that the ore-bearing host rocks in the Hongtoushan deposit erupted from 2.59 to 2.51 Ga and then underwent metamorphism from 2.52 to 2.47 Ga. The emplacement and metamorphic events of volcanic rocks were almost continuous, which corresponds with the widespread thermal events at 2.5 Ga in the North China Craton.
In the age histograms (Figure 18B,D), the U-Pb zircon ages of the host rocks display a peak at about 2.52–2.5 Ga, one Hf isotope single-stage model age (TDM1) peak at about 2.6–2.52 Ga, and two Hf isotope two-stage model age (TDM2) peaks at about 2.62–2.52 Ga and 2.7–2.65 Ga, respectively (Figure 18). The first peak of the two-stage model ages (TDM2) almost coincides with the peak of the single-stage model ages (TDM1), which suggests a short residence time of the parent rocks in the crust and the differentiation of the crust and mantle at about 2.520–2.6 Ga. This corresponds to the ~2.62.5 Ga crustal growth event in the North China Craton that was identified in previous studies [67,68,69]. It is worth noting that we observed another two-stage model age peak at around 2.8–2.7 Ga, which corresponds to another juvenile crust-forming period for the North China Craton [70].
In our research, all of the zircons have relatively high, positive ε Hf(t) values (3.07–10.45). The two types of host rocks all have higher Hf TDM1 ages than formation ages; this may indicate that the magma source region is contaminated by crustal material or originates from an enriched mantle [71]. In the ε Hf(t) versus U-Pb age diagram (Figure 18A), most samples fall between the depleted mantle and chondrite evolution lines, while a few fall above the depleted mantle. In the   176 Hf/   177 Hf versus   207 Pb/   206 Pb diagram Figure 18B, almost all the zircons show relatively higher initial (   176 Hf/   177 Hf)i ratios than the depleted mantle and are distributed between the enriched mantle array and the depleted mantle array. Part of the samples are plotted in the scope of known modern plumes. When combining the discussion of host rock geochemistry, limited crustal contamination is the conclusion. Thus, the relatively high ε Hf(t) values should come from an enriched mantle source. With the evidence above, this points to a mantle-plume-related event that closely corresponds to volcanism during the ~2.5 Ga mantle plume event, which was global in its extent [72,73].
The formation and preservation of the VMS deposits is influenced by numerous factors such as the source of the metals and sulfur, the tectonic setting, and the ore-forming processes. One of the most important factors is a large stable heat source that can drive a long-lived, high-temperature convective hydrothermal system and has enough permeability to allow for hydrothermal circulation and discharge [62,63].
Based on the geochemistry and chronology results of the ore-bearing host rocks, we are more considerate that the host rocks of the Hongtoushan VMS deposit were generated under a rift environment that was driven by Archean mantle plume activity at 2.6–2.5 Ga. Under the continuous action of the mantle plume, a large amount of mantle-derived magma rose up and caused the partial melting and thinning of the crust, ultimately leading to the formation of rifts and the extensive eruption of volcanic rocks at the seafloor. Due to the good preservation of the VMS deposits, we can say that the rift extensional environment allowed fluid to flow down to the deeper part of the crust and, thus, increase the volume of leaching metals [59]. The subsequent metamorphic deformation brought about structural changes in the primary VMS ore bodies and caused the migration and enrichment of metallic elements, thus forming the ore pillar.
Figure 18. (A) Zircon ε Hf(t) versus zircon age from the Hongtoushan deposit; the depleted mantle reference lines are from Griffin et al. (2000) [74], and the crustal evolution lines are from Wan et al., 2013 [75]. (B)   176 Hf/   177 Hf versus   207 Pb/   206 Pb diagram modified from Zhu et al. (2017) [67]; the line of chondrite is from Blichert-Toft and Albarède (1997) [76], and the fields of depleted mantle and modern known plumes are from Nowell et al. (1998) [77]. (C) Hf isotope TDM1 and TDM2 age histogram of amphibole plagioclase gneiss from the Hongtoushan VMS deposit. (D) Hf isotope one-stage and two-stage modal age histograms of biotite plagioclase gneiss from the Hongtoushan VMS deposit.
Figure 18. (A) Zircon ε Hf(t) versus zircon age from the Hongtoushan deposit; the depleted mantle reference lines are from Griffin et al. (2000) [74], and the crustal evolution lines are from Wan et al., 2013 [75]. (B)   176 Hf/   177 Hf versus   207 Pb/   206 Pb diagram modified from Zhu et al. (2017) [67]; the line of chondrite is from Blichert-Toft and Albarède (1997) [76], and the fields of depleted mantle and modern known plumes are from Nowell et al. (1998) [77]. (C) Hf isotope TDM1 and TDM2 age histogram of amphibole plagioclase gneiss from the Hongtoushan VMS deposit. (D) Hf isotope one-stage and two-stage modal age histograms of biotite plagioclase gneiss from the Hongtoushan VMS deposit.
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8. Conclusions

(1)
The ore-bearing host metamorphic rocks in the Hongtoushan VMS deposit show a continuous variation in composition, with amphibole plagioclase gneiss having a protolith of basalt and the biotite plagioclase gneiss having a protolith of andesite to rhyolite, indicating a volcanic cycle from basic to medium-acidic volcanic rocks.
(2)
The amphibole plagioclase gneiss of the Hongtoushan deposit has a composition resembling contaminated ocean plateau basalt (OPB), which is generally interpreted as being generated from the mantle plume head.
(3)
The petrogenesis of the biotite plagioclase gneiss in the Hongtoushan VMS deposit is interpreted as crustal assimilation combined with the fractional crystallization of basic magma (the magma source of the amphibole plagioclase gneiss) in a rift environment.
(4)
The zircon geochronology indicates that the ore-bearing host rocks in the Hongtoushan deposit were generated between 2.59 and 2.51 Ga, followed by a metamorphic event spanning from 2.52 to 2.47 Ga. The continuous emplacement of volcanic rocks and subsequent metamorphic processes correspond to the 2.5 Ga regional plume-related thermal events of the North China Craton.
(5)
The tectonic setting of the Hongtoushan VMS deposit might be more reasonable due to the rift settings that are related to the ~2.5 Ga global mantle plume activities. The stretching environment provided by rift structures and the high-temperature heat source from the mantle plume activity created ideal conditions for long-term hydrothermal reactions and heat sources, contributing to the formation of the large VMS deposits.

Author Contributions

Conceptualization and writing—original draft preparation, X.Y.; writing—review, editing, and supervision, E.W.; methodology and software, Y.M. and J.F.; validation, K.S. and S.M. All authors have read and agreed to the published version of the manuscript.

Funding

This work was financially supported by the National Natural Science Foundation of China (Grant Number 41372098) and the Fundamental Research Funds for the Central Universities (Grant Number N2123030).

Data Availability Statement

The original contributions presented in the study are included in the article.

Acknowledgments

We thank Beijing GeoAnalysis Co., Ltd., Beijing, China; the Geoanalytical Center of Nuclear Industry in Beijing; the Institute of Geology and Geophysics, Chinese Academy of Sciences (IGGCAS) in Beijing; and Createch Testing Technology Co., Ltd., Beijing for their valuable services and assistance in the data testing conducted for this article. We also thank the Hongtoushan Cu-Zn deposit for their kind help in the field investigations and sampling.

Conflicts of Interest

The authors declare no conflicts of interest.

Abbreviations

The following abbreviations are used in this manuscript:
VMSVolcanogenic massive sulfide
QGBQingyuan granitic-greenstone belt
NCCNorth China Craton
REERare earth element
HREEHeavy rare earth element
LREELight rare earth element
LILEsLarge-ion lithophile elements
HFSEsHigh-field-strength elements
OIBOcean island basalt
OPBOcean plateau basalt
ARCArc volcanic rock
AFCAssimilation and fractional crystallization

Appendix A

Table A1. In situ zircon U-Pb isotopic dating data for the ore-bearing metamorphic rocks from the Hongtoushan VMS deposit.
Table A1. In situ zircon U-Pb isotopic dating data for the ore-bearing metamorphic rocks from the Hongtoushan VMS deposit.
Rock TypeAmphibole Gneiss
Point No.SizeIsotopic RatioIsotopic Age (Ma)
μ m   207 Pb/   206 Pb1 σ   207 Pb/   235 U1 σ   206 Pb/   238 U1 σ   207 Pb/   206 Pb1 σ   207 Pb/   235 U1 σ   206 Pb/   238 U1 σ Th (ppm)U (ppm)Th/U
HTS-1605-2-00100×400.17420.004411.260.350.46800.012025814025352624774852.0084.500.615
HTS-1605-2-0180×600.16970.003211.470.250.49240.009325513025562025784114.10120.700.117
HTS-1605-2-0280×350.16750.004110.450.260.46100.009125224224752224424135.10123.800.284
HTS-1605-2-03120×500.17250.003510.930.230.46540.007625723425161924613465.70135.400.485
HTS-1605-2-0480×300.17520.00311.380.200.48030.0077260627255216252734215.00197.001.091
HTS-1605-2-0580×400.16720.002310.410.130.45860.0059252924247012243226267.00373.000.716
HTS-1605-2-0660×400.17020.00310.690.220.46320.0079255329249519245135123.70192.000.644
HTS-1605-2-0780×500.17070.005410.850.310.47400.015025555125072724966517.00158.000.108
HTS-1605-2-0880×350.16250.003810.410.210.47600.008724893524691825083814.30197.000.073
HTS-1605-2-09100×400.16830.001910.870.150.47630.0073253719251212251032144.60260.000.556
HTS-1605-2-1090×400.16550.003610.290.200.46170.00732504372458182446333.66192.500.019
HTS-1605-2-1175×400.16740.002311.230.200.48000.0065252823254315252529128.00271.000.472
HTS-1605-2-1250×300.16620.002510.400.150.46210.007025152524691324473160.10260.000.231
HTS-1605-2-1360×450.16440.002310.930.220.47950.008825042525131925213826.80181.000.148
HTS-1605-2-1475×500.16860.003510.510.300.45900.010025313624712124314316.00160.000.100
HTS-1605-2-1590×400.16070.00529.990.350.45210.009724266424363224004423.5097.000.242
HTS-1605-2-1660×300.16850.003411.010.260.47320.008125343525202125003718.7098.100.191
HTS-1605-2-17100×450.16850.003210.530.240.46050.00942535322478212439422.20129.000.017
HTS-1605-2-18100×350.16960.003410.680.230.45710.008425403324922024233740.4080.300.503
HTS-1605-2-1960×300.16950.003110.550.230.45820.008425483024792024343535.00125.300.279
HTS-1605-6-0285×350.165140.001811.630.230.51050.0095250919257519265941113.95387.510.294
HTS-1605-6-06100×350.166910.001711.160.180.48460.0075252817253715254733106.84363.720.294
HTS-1605-6-0780×400.167470.001911.240.210.48670.009025321925431725563988.35769.970.115
HTS-1605-6-0980×500.168070.001611.280.180.48640.0074253915254715255532129.021118.180.115
HTS-1605-6-1160×400.168230.001710.760.170.46300.006525401725031524532988.74435.520.204
HTS-1605-6-1390×400.167720.001510.480.190.45230.0073253515247816240532134.00714.810.187
HTS-1605-6-1490×350.168030.001510.710.190.46210.0078253815249916244934219.04403.680.543
HTS-1605-6-1545×350.166920.001611.070.190.48010.006725271025291625282976.78553.580.139
HTS-1605-6-1680×300.167550.001610.520.160.45490.0058253316248214241726158.16496.830.318
HTS-1605-6-1790×500.164800.001810.380.170.45650.0062250518246915242427136.93556.670.246
HTS-1605-6-1880×450.165970.001610.300.200.44980.0075251849246218239433100.78428.990.235
HTS-1605-6-1960×400.164730.001910.320.220.45430.008525051824642024143884.38261.330.323
HTS-1605-6-2080×400.166490.001810.420.170.45380.0065252417247215241229153.94524.920.293
HTS-1605-9-19130×400.16410.002510.550.180.46030.007924992524791624423310.20233.000.044
HTS-1605-9-29100×450.16620.002411.250.220.48980.00752512252541182567326.35125.400.051
HTS-1605-9-27100×250.16430.002310.480.140.45910.006324972324761324332810.19154.600.066
HTS-1605-9-5110×500.16630.002312.020.420.51300.014025292326042826645726.00430.000.060
HTS-1605-9-18100×450.16950.002510.360.210.43890.008725542324641923413930.30151.100.201
HTS-1605-9-11100×350.17070.004511.930.360.49300.011025605025882525794512.70103.000.123
HTS-1605-9-24105×400.16540.004110.560.360.46400.011024944524852924524711.3088.100.128
HTS-1605-9-26130×200.17170.002810.860.200.45660.007925652725071724213518.07110.300.164
HTS-1605-9-13100×250.16920.002810.870.190.46070.006125442725091724412720.7896.400.216
HTS-1605-9-4110×350.16730.001911.400.170.48820.005925282025531425612552.50162.000.324
HTS-1605-9-16120×300.17040.004512.350.360.50700.012025375026202926655415.3242.400.361
HTS-1605-9-15100×350.17020.004210.910.250.46270.009125604325192124533927.6077.200.358
HTS-1605-9-2150×450.16690.001110.900.130.46780.0050252411251310247322272.00646.000.421
HTS-1605-9-25100×350.18830.006313.350.470.51400.012026835626873326665316.1636.100.448
HTS-1605-9-20120×500.17460.004311.200.300.46500.012025883925302524525419.3044.800.431
HTS-1605-9-28100×250.17250.002011.250.140.46990.0055257719254211248124124.40212.000.587
HTS-1605-9-10100×500.1670.003510.960.290.47500.012025153425192325104639.3066.900.587
HTS-1605-9-12100×350.1720.005010.830.230.45290.0080256140251319241034152.00168.000.905
HTS-1605-9-17100×400.16350.00139.520.090.41260.00402492122388.18.4222618978.001039.000.941
HTS-1605-1-0170×350.16160.001510.130.100.45290.003724701624459.6240717115.00532.000.216
HTS-1605-1-0270×350.16100.001710.630.120.47770.00422462182490102516187.60421.000.018
HTS-1605-1-0380×300.16280.002210.030.130.45020.0046248123243612239620152.00486.000.313
HTS-1605-1-0460×400.16150.001710.400.140.47050.004924681824691224852115.00479.000.031
HTS-1605-1-0590×400.16100.001010.690.080.47830.00342466112495.76.825191517.801001.000.018
HTS-1605-1-0660×350.16170.001310.510.080.46950.00342470132480.17.424811510.34697.000.015
HTS-1605-1-0780×500.16060.001210.320.110.46380.004624591224621024552017.40988.000.018
HTS-1605-1-0870×400.16120.001211.040.100.49510.00342466122525.58.525921520.20689.000.029
HTS-1605-1-0960×300.16140.002610.130.170.45830.005124672824451624322322.90576.000.040
HTS-1605-1-1060×300.16050.001410.630.090.48100.00382459152490.68.125311723.00851.000.027
HTS-1605-1-1190×450.16110.00119.940.100.44700.00422466122428.39.523811919.40949.000.020
HTS-1605-1-1260×400.16130.00199.960.130.44910.0054246621242812239024175.00400.000.438
HTS-1605-1-1360×350.16130.001010.150.100.45330.00322468102447.58.724101418.041269.000.014
HTS-1605-1-1460×350.16020.001410.010.100.45050.004324541624348.823991920.50643.000.032
HTS-1605-1-1590×500.16150.001410.350.090.46360.00352468142467.78.924551519.55678.000.029
HTS-1605-1-1680×350.16110.00159.940.110.45200.005524661524291024042425.702060.000.012
HTS-1605-1-1760×300.16230.001810.380.120.46310.00582477192467112451257.61385.000.020
HTS-1605-1-1860×400.16080.001410.430.100.46930.004224611424728.724801824.30851.000.029
HTS-1605-1-1975×400.16120.001210.290.120.45870.004424671324591024331926.00775.000.034
HTS-1605-3-0140×300.16500.001910.750.230.47230.00912507202502192494408.60493.840.017
HTS-1605-3-0280×250.16580.001810.580.210.46280.008925165124871924523914.75611.730.024
HTS-1605-3-03110×400.16570.001611.060.240.48400.010125151725282025454433.02725.030.046
HTS-1605-3-0450×400.16600.001510.830.160.47270.00612518152508132495277.00551.710.013
HTS-1605-3-0760×250.16440.001910.430.210.45990.00922502192473192439418.73403.070.022
HTS-1605-3-1070×300.16660.002011.390.190.49590.00752524202556152596325.57447.620.012
HTS-1605-3-1160×400.16390.001710.920.180.48320.007324961725171525413225.52862.380.030
HTS-1605-3-1240×350.16610.001511.220.210.48950.00862520482542182568375.04483.950.010
HTS-1605-3-1390×400.16390.002010.710.250.47380.01042496212499222500454.61391.940.012
HTS-1605-3-1490×400.16330.001610.450.160.46400.006225001724761424572726.38715.330.037
HTS-1605-3-1570×500.16400.001610.820.170.47780.006724981525071525182948.23845.550.057
HTS-1605-3-1640×300.16480.001710.500.140.46200.00572506182480122448252.28485.960.005
HTS-1605-3-1760×350.16420.001510.440.150.46080.005724991724751324432511.96606.900.020
HTS-1605-3-1840×250.16490.001810.370.230.45610.009725061924692024224312.221200.060.010
HTS-1605-3-1990×400.16510.001710.750.170.47190.006325091725021424922815.85522.460.030
HTS-1605-8-0040×300.16200.001010.140.100.45200.005424741124469.224022468.20543.000.126
HTS-1605-8-0140×250.16160.001510.090.100.45250.003924691624428.924051727.9056.000.498
HTS-1605-8-0375×400.16630.001610.150.120.44640.005525181624491023782439.0082.100.475
HTS-1605-8-0480×350.16540.001610.110.110.44130.005725071624439.623582573.60122.600.600
HTS-1605-8-0560×500.16180.001510.560.130.46430.004724701624831124572058.60116.900.501
HTS-1605-8-0670×450.16510.001310.190.100.44790.004925061324518.923882154.10108.500.499
HTS-1605-8-0740×300.16350.001410.040.090.44550.004924921524378.523742250.00461.000.108
HTS-1605-8-0860×450.16420.003210.240.220.45460.007324913324512024133374.70535.000.140
HTS-1605-8-0970×500.16700.003610.260.250.44870.009525183524542323854236.3086.300.421
HTS-1605-8-1040×250.16470.002810.780.240.46970.008525032725052024843535.1084.800.414
HTS-1605-8-1140×300.16340.003310.290.210.45740.008424753524571924243752.5098.200.535
HTS-1605-8-1340×250.16480.003510.200.220.45250.009524923524472024024221.2048.100.441
HTS-1605-8-1460×400.16420.00309.990.170.44700.007324913024331723803335.6071.600.497
HTS-1605-8-1570×400.16390.003510.090.220.45020.007224883524372023943243.70100.900.433
HTS-1605-8-1640×250.16570.003510.600.220.46390.007625033524831924543463.80487.000.131
HTS-1605-8-1780×500.16990.004710.880.320.47000.011025504325072624764954.90125.200.438
HTS-1605-8-1840×300.16050.003610.500.290.46270.0090244940247824244940107.70220.800.488
HTS-1605-8-1970×400.16280.002910.030.160.45650.006524773024351524232948.8096.700.505
HTS-1605-8-260×500.16400.003010.160.210.45120.007924873124471923983528.5772.700.393
HTS-1605-8-2060×450.16750.003810.060.250.44550.0087252138243824237339333.20285.101.169
HTS-1605-8-2170×400.16270.004010.360.320.45600.010024794224612924164450.3099.900.504
HTS-1605-8-2260×450.16500.003010.380.180.45620.006524963024671624252928.9059.500.486
HTS-1605-8-2360×400.16460.003710.350.250.45710.007924883724592224293640.4088.900.454
HTS-1605-8-2560×500.16350.003510.200.240.45440.008724783624502124113996.10844.000.114
HTS-1605-8-2640×300.16570.003210.130.220.44580.008125093324442123743646.1077.900.592
HTS-1605-8-2770×300.16250.00419.800.260.44080.009424754524082423504260.60454.000.133
HTS-1605-8-2840×300.16650.002210.490.160.45540.0058251622247614241726232.00228.001.018
HTS-1605-8-2950×400.16620.002010.050.140.44060.005925142124391323522631.4091.200.344
Table A2. In situ zircon Lu-Hf isotopic dating data for ore-bearing metamorphic rocks from the Hongtoushan VMS deposit.
Table A2. In situ zircon Lu-Hf isotopic dating data for ore-bearing metamorphic rocks from the Hongtoushan VMS deposit.
Rock TypeAmphibole Plagioclase Gneiss
Point No.   176 Hf/   177 Hf(corr)2 σ   176 Yb/   177 Hf(corr)2 σ   176 Lu/   177 Hf(corr)2 σ Age (Ma)Hf(I) ε Hf(t)2 σ T(DM)1T(DM)2
HTS-1605-2-000.2814620.0000220.0908150.0021010.0032160.00006025810.2813032776.300.772654.972692.22
HTS-1605-2-010.2815320.0000190.1032080.0004380.0032390.00001325510.2813740718.110.692555.062557.10
HTS-1605-2-020.2815120.0000150.0872150.0020070.0028380.00005625220.2813756447.490.552555.072572.25
HTS-1605-2-030.2813910.0000150.0529620.0006780.0017960.00001825720.2813030956.080.552652.802698.39
HTS-1605-2-040.2814540.0000200.0915070.0024880.0032920.00009026060.2812894346.390.722672.882706.35
HTS-1605-2-050.2814420.0000120.0456850.0007940.0017200.00002225290.2813586667.050.442577.362604.81
HTS-1605-2-060.2814690.0000180.0763650.0043510.0025070.00008725530.2813464757.180.632594.082616.02
HTS-1605-2-070.2814800.0000170.1068800.0006990.0036200.00002525550.2813029285.680.592659.042709.64
HTS-1605-2-080.2814450.0000160.0518040.0015890.0017430.00005124890.2813616156.220.552575.192624.02
HTS-1605-2-090.2813810.0000130.0392160.0005190.0013890.00001925370.2813137665.640.452638.522697.57
HTS-1605-2-100.2816220.0000240.1482140.0043110.0051100.00010725040.2813775527.140.862557.162579.62
HTS-1605-2-120.2814030.0000160.0726520.0023010.0023730.00004725150.2812889434.240.562677.852765.73
HTS-1605-2-130.2815230.0000190.1027400.0022310.0033200.00007425040.2813638986.650.682574.322609.42
HTS-1605-2-140.2814920.0000190.1037510.0087300.0030930.00020825310.2813423116.510.692602.712639.20
HTS-1605-2-150.2814900.0000210.1074430.0009980.0032770.00003024260.2813380763.910.752619.012715.70
HTS-1605-2-160.2813980.0000180.0743080.0007210.0024300.00001825340.2812803484.380.642689.002772.27
HTS-1605-2-170.2815240.0000200.1212140.0018800.0039940.00004925350.2813299466.170.692622.452663.59
HTS-1605-2-180.2815030.0000170.0970700.0012070.0029610.00003025400.2813588897.310.622577.822597.27
HTS-1605-2-190.2816600.0000200.1396380.0009480.0044810.00003425480.28144177610.450.712453.572411.13
HTS-1605-6-010.2814360.0000200.0808290.0002490.0025000.00001025180.2813154025.240.702640.692706.44
HTS-1605-6-020.2814690.0000150.0819370.0007560.0027570.00003425090.281337235.820.542611.012664.40
HTS-1605-6-030.2814970.0000150.0759770.0004810.0026330.00002125160.2813708277.190.532562.172586.38
HTS-1605-6-060.2814110.0000150.0606280.0017780.0018820.00005025280.2813204885.660.552630.982688.84
HTS-1605-6-070.2813600.0000190.0450300.0005380.0016690.00003325320.2812790384.300.672687.692776.15
HTS-1605-6-080.2814210.0000140.0570820.0006100.0018650.00001525150.2813310495.730.482616.872674.33
HTS-1605-6-090.2815470.0000170.1029520.0016620.0032010.00005525390.2813916468.450.602530.682526.70
HTS-1605-6-110.2815480.0000150.1103310.0015830.0034150.00004425400.2813818958.140.542544.692546.80
HTS-1605-6-120.2814720.0000150.0690060.0011830.0023290.00003725390.2813588897.290.542577.232597.99
HTS-1605-6-130.2814630.0000160.0711770.0008010.0023260.00001225350.2813504276.890.562589.452619.02
HTS-1605-6-140.2814300.0000160.0568750.0012560.0018760.00003025380.281338996.560.582604.602641.98
HTS-1605-6-150.2815180.0000170.0911190.0005370.0029720.00001925270.2813740467.550.592557.092572.63
HTS-1605-6-160.2814280.0000190.0670720.0012890.0021700.00003625330.2813228555.870.662628.162680.32
HTS-1605-6-170.2814480.0000170.0754710.0012360.0023190.00003125050.2813371285.730.592610.152667.00
HTS-1605-6-180.2814130.0000130.0447290.0003590.0016140.00001025180.2813357155.970.462609.562662.18
HTS-1605-6-200.2813830.0000140.0330600.0010120.0010800.00002825240.2813307885.940.512614.802668.76
HTS-1605-9-020.2814120.0000180.0697710.0009360.0021970.00002725240.2813056355.050.622653.022723.62
HTS-1605-9-170.2814340.0000140.0600280.0002420.0020240.00001224920.2813373715.430.492609.702674.96
HTS-1605-9-240.2814230.0000190.0578810.0004080.0021510.00002424940.2813199944.850.662634.442711.56
HTS-1605-9-270.2814730.0000150.0705600.0033660.0022220.00010224970.2813670136.600.532568.222607.11
Rock TypeBiotite Plagioclase Gneiss
Point No.   176 Hf/   177 Hf(corr)2 σ   176 Yb/   177 Hf(corr)2 σ   176 Lu/   177 Hf(corr)2 σ Age (Ma)Hf(I) ε Hf(t)2 σ T(DM)1T(DM)2
HTS-1605-1-000.2813550.0000170.0027480.0000530.0000920.00000324700.281355.400.612585.492659.07
HTS-1605-1-020.2813520.0000140.0025090.0000730.0000740.00000324620.281355.110.512589.372670.62
HTS-1605-1-030.2813440.0000140.0106100.0000650.0003370.00000324810.281334.820.492617.732703.41
HTS-1605-1-040.2813420.0000210.0057980.0001020.0001820.00000424680.281334.730.742609.282698.74
HTS-1605-1-050.2813010.0000190.0026940.0000780.0000890.00000324660.281303.360.682658.422781.03
HTS-1605-1-060.2813760.0000140.0025920.0000530.0000840.00000224700.281376.140.482557.852613.85
HTS-1605-1-070.2813090.0000130.0033500.0002870.0001110.00001124590.281303.460.462648.642769.29
HTS-1605-1-080.2814070.0000200.0283190.0008340.0009940.00003024660.281365.620.712576.312642.33
HTS-1605-1-090.2813860.0000170.0093670.0006080.0002940.00001924670.281376.070.612558.372615.79
HTS-1605-1-100.2813620.0000130.0027330.0000910.0000790.00000324590.281365.390.462576.302651.10
HTS-1605-1-110.2813900.0000150.0124720.0000550.0004330.00000224660.281375.980.542561.272620.58
HTS-1605-1-120.2813090.0000180.0024730.0000650.0000760.00000224660.281313.670.642646.612761.80
HTS-1605-1-130.2813030.0000170.0027440.0000760.0000790.00000324680.281303.510.602654.292773.08
HTS-1605-1-140.2813180.0000120.0037970.0001050.0001010.00000324540.281313.680.422635.922751.74
HTS-1605-1-150.2813540.0000140.0035520.0000870.0001040.00000324680.281355.290.492587.892664.21
HTS-1605-1-160.2813270.0000110.0020830.0000390.0000560.00000224660.281324.370.382620.552719.25
HTS-1605-1-170.2813460.0000200.0040760.0000820.0001510.00000324770.281345.140.702601.402680.35
HTS-1605-1-190.2813850.0000160.0138230.0002180.0004540.00000624670.281365.790.582569.242632.80
HTS-1605-3-010.2814250.0000170.0071690.0000210.0003260.00000225070.281418.330.622508.142508.79
HTS-1605-3-020.2813930.0000240.0787930.0008690.0028590.00002625160.281263.070.842728.022838.15
HTS-1605-3-030.2814400.0000200.0153780.0000590.0006800.00000325150.281418.450.702510.042507.31
HTS-1605-3-040.2814230.0000190.0210870.0000730.0010000.00000525180.281377.360.682554.452576.51
HTS-1605-3-050.2814040.0000200.0378210.0023670.0015100.00009424940.281335.300.722614.782684.33
HTS-1605-3-060.2814050.0000220.0118520.0002440.0005270.00001225060.281387.250.772547.642573.66
HTS-1605-3-070.2813450.0000160.0099820.0001870.0004380.00000825020.281325.170.562622.612697.95
HTS-1605-3-080.2814460.0000210.0125330.0000980.0004990.00000525220.281429.160.742489.972469.98
HTS-1605-3-090.2814370.0000250.0150860.0000530.0005820.00000425390.281419.060.902508.472489.54
HTS-1605-3-100.2813820.0000160.0114790.0001140.0004680.00000325240.281366.970.552574.372605.79
HTS-1605-3-110.2814020.0000190.0137700.0000690.0006580.00000424960.281376.700.692560.472599.99
HTS-1605-3-120.2814340.0000190.0807790.0009000.0033890.00003225200.281273.720.662708.362801.63
HTS-1605-3-130.2814360.0000170.0152010.0003000.0005540.00000824960.281418.080.602507.852515.17
HTS-1605-3-140.2814330.0000180.0139120.0001960.0005480.00000525000.281418.090.642510.982517.76
HTS-1605-3-150.2814360.0000170.0111470.0002230.0004760.00000424980.281418.260.612502.672505.66
HTS-1605-3-160.2814080.0000180.0075580.0000490.0003330.00000325060.281397.700.632530.892546.58
HTS-1605-3-170.2814490.0000190.0103150.0002550.0004240.00000724990.281438.850.672481.512470.57
HTS-1605-3-180.2814510.0000200.0124480.0001530.0005410.00000825060.281438.900.702486.012473.36
HTS-1605-8-030.2814230.0000190.0182480.0002720.0008630.00001525030.281387.270.682545.102570.54
HTS-1605-8-040.2813820.0000160.0134370.0001230.0005320.00000425090.281366.510.552578.642621.70
HTS-1605-8-050.2814020.0000190.0112380.0000520.0004900.00000324960.281386.990.692549.402582.51
HTS-1605-8-060.2814340.0000190.0105050.0001710.0004630.00001024870.281417.970.662504.232514.93
HTS-1605-8-080.2814360.0000170.0101520.0000480.0004140.00000125060.281428.550.602498.842494.38
HTS-1605-8-090.2814330.0000180.0164390.0000900.0006610.00000424920.281407.720.642518.352534.49
HTS-1605-8-120.2814360.0000170.0176080.0014140.0005890.00003724920.281417.930.612509.982521.05
HTS-1605-8-150.2814080.0000180.0071440.0001060.0003110.00000825030.281397.670.632529.482546.10
HTS-1605-8-170.2814490.0000190.0218320.0016280.0008030.00004724910.281418.020.672505.932514.98
HTS-1605-8-230.2814510.0000200.0130190.0002960.0005700.00001024880.281428.420.702487.892487.82
HTS-1605-8-290.2814230.0000190.0116920.0000570.0005020.00000224910.281407.610.682521.412540.26
Table A3. Major (wt%) element compositions and trace (rare earth) element (ppm) compositions of the ore-bearing metamorphic rocks from the Hongtoushan VMS deposit.
Table A3. Major (wt%) element compositions and trace (rare earth) element (ppm) compositions of the ore-bearing metamorphic rocks from the Hongtoushan VMS deposit.
Rock TypeAmphibole Plagioclase Gneiss
No.Al   2 O   3 BaOCaOCr   2 O   3 Fe   2 O   3 TK   2 OMgOMnONa   2 OP   2 O   5 SiO   2 SrOTiO   2 LOITotal
HTSI-915.380.033.020.0210.252.975.150.102.270.1956.530.010.603.0999.60
HTSI-1116.670.028.650.028.750.345.000.133.540.1055.400.010.520.7299.87
HTSM-116.340.037.070.019.920.993.900.143.710.2354.750.020.851.8499.80
HTSM-415.990.027.82<0.0112.560.643.170.193.460.1853.100.021.211.5499.90
HTSM-814.250.048.340.0213.210.935.260.203.760.3447.850.042.443.1999.86
HTSM-914.810.0311.570.0612.580.947.420.222.490.0547.630.030.681.3799.88
No.LaCePrNdSmEuGdTbDyHoErTmYbLuCo
HTSI-911.2022.502.6210.402.300.582.140.352.060.411.150.181.060.1630.60
HTSI-116.8014.501.898.001.940.681.990.362.070.451.310.201.390.2027.80
HTSM-112.1030.804.4119.704.521.074.230.673.960.812.310.352.350.3630.90
HTSM-46.5018.302.6912.603.601.234.480.764.701.033.110.462.910.4534.50
HTSM-828.3065.809.2239.408.812.668.651.287.061.453.690.503.210.4635.00
HTSM-97.5020.803.1213.904.030.793.650.634.000.852.350.342.360.3747.70
No.NiCuZrSrYZnCsBaPbUVCrRbGaHf
HTSI-950.3055.0039.80118.509.70366.004.93216.0035.900.28103.00122.00105.2516.301.05
HTSI-1177.8010.9048.10154.0012.6077.000.2059.302.500.22165.0075.003.5516.201.40
HTSM-145.4033.0069.80233.0021.6078.000.37198.003.600.13178.0061.0042.7019.852.00
HTSM-434.1026.80109.00178.0026.00155.000.3280.001.700.20229.0020.0013.1019.403.00
HTSM-857.3033.10267.00374.0036.40131.000.48277.003.000.40245.00180.0034.6025.306.50
HTSM-9130.0067.1029.15264.5021.95222.000.35143.006.900.22245.00203.0012.5518.951.15
No.TaThNbPTiK Σ REE Σ LREE Σ HREE δ Eu δ Ce(La:Sm)   N (La:Yb)   N (Sm:Nd)   N (Gd:Yb)   N
HTSI-90.302.126.30860.003597.0024,654.8657.1149.607.510.790.973.067.120.681.63
HTSI-110.220.743.35450.003117.402822.4441.7833.817.971.050.962.203.300.751.16
HTSM-10.260.664.95990.005095.758218.2987.6472.6015.040.741.011.683.470.711.45
HTSM-40.310.504.80790.007253.955312.8362.8244.9217.900.941.051.141.510.881.24
HTSM-81.303.7621.201490.0014,627.807720.21180.49154.1926.300.920.982.025.940.692.17
HTSM-90.330.485.00220.004076.607803.2264.6950.1414.550.621.031.172.140.891.25
Rock TypeBiotite-Rich Gneiss
No.Al   2 O   3 BaOCaOCr   2 O   3 Fe   2 O   3 TK   2 OMgOMnONa   2 OP   2 O   5 SiO   2 SrOTiO   2 LOITotal
HTSF-16.940.051.030.012.421.440.330.021.930.0584.42<0.010.160.9399.73
HTSF-29.530.012.08<0.012.271.020.540.023.330.0378.92<0.010.102.0699.93
HTSF-411.630.010.77<0.012.140.741.340.025.190.0977.360.010.120.63100.05
HTSF-512.750.061.45<0.011.642.290.400.024.460.0275.210.010.121.67100.10
HTSF-1014.000.023.14<0.012.800.901.060.023.940.0572.280.010.271.2499.73
HTSF-1113.330.281.71<0.012.482.910.450.024.160.2572.190.010.211.0399.03
HTSF-1414.300.082.340.024.092.432.190.064.140.1068.550.040.281.40100.00
HTSF-1515.920.033.040.012.821.321.050.025.120.1668.530.050.281.4499.79
HTSF-1614.860.033.53<0.015.511.021.530.084.540.0766.800.040.401.4099.83
HTSF-1715.740.082.980.014.591.861.750.074.660.1866.010.080.411.68100.10
HTSF-1816.460.052.700.013.321.211.820.045.850.1965.820.080.551.7499.84
HTSF-1914.330.092.280.014.133.591.610.053.770.1565.560.040.343.9099.85
HTSI-113.580.042.220.016.762.543.660.113.120.0464.640.010.471.9099.09
HTSI-214.910.114.840.045.222.624.790.074.170.2059.840.070.612.3699.85
No.LaCePrNdSmEuGdTbDyHoErTmYbLuCo
HTSF-15.2010.901.354.901.130.301.120.170.760.110.280.030.180.043.00
HTSF-229.1052.405.9820.403.450.552.820.492.900.601.660.271.650.272.80
HTSF-428.2060.606.7828.206.001.456.691.196.741.494.150.674.050.703.90
HTSF-519.6032.403.099.701.600.491.330.160.850.150.370.070.360.052.60
HTSF-103.606.800.752.800.720.580.660.110.610.130.390.050.430.086.80
HTSF-1115.2031.903.9815.703.710.893.610.582.670.410.840.110.510.083.00
HTSF-1425.6043.604.5414.802.050.601.410.181.070.220.560.090.670.1011.80
HTSF-1517.1032.603.4111.701.520.500.760.090.350.060.150.030.190.027.40
HTSF-1612.4025.303.0811.702.610.612.620.482.970.652.050.352.570.4610.90
HTSF-1726.0056.206.3423.604.331.062.960.401.950.400.970.140.840.1311.20
HTSF-187.4013.701.565.500.820.550.500.060.260.050.130.020.160.0211.90
HTSF-1937.9073.007.5626.204.010.832.620.351.900.381.080.150.960.169.50
HTSI-134.5078.709.8238.809.021.229.851.7510.552.366.850.996.580.9614.20
HTSI-222.7041.904.4917.103.420.922.500.361.940.401.080.150.880.1519.90
No.NiCuZrSrYZnCsBaPbUVCrRbGaHf
HTSF-14.0027.5088.0047.303.2065.000.80358.004.200.3013.0070.0023.708.562.40
HTSF-22.9035.50144.5564.7014.4044.000.4878.704.700.169.0049.0025.009.843.60
HTSF-42.1024.50225.0062.008.2094.000.57110.0034.300.5024.0020.0014.1013.257.00
HTSF-52.408.70104.00110.503.5022.000.91520.003.800.3013.0020.0054.1012.453.50
HTSF-107.2028.70243.00132.503.60123.002.17124.004.400.3045.0050.0038.1014.356.50
HTSF-113.904.50144.00135.0011.3066.000.612810.0010.100.7016.0050.0040.6013.253.60
HTSF-1439.909.0080.15357.005.9057.003.04652.5013.202.0851.00151.0085.7019.152.20
HTSF-1510.8014.9089.75485.001.5538.002.07168.758.500.3131.0046.0065.2518.702.30
HTSF-1612.502.90127.00387.0021.1066.000.51277.003.200.3076.0050.0033.5016.253.10
HTSF-1716.308.3078.95677.509.70101.001.25652.509.800.2263.0048.0051.3520.202.05
HTSF-1842.109.90102.05723.001.3561.001.05468.507.900.3842.0061.0031.3520.902.40
HTSF-1925.7010.70100.80415.508.9564.007.32784.0012.100.7852.0061.00109.2518.802.70
HTSI-133.2080.40245.0099.5067.40585.003.68337.009.903.3075.0060.0092.4020.006.60
HTSI-2131.5033.60133.25596.0010.5062.000.64882.5026.701.2894.00196.0053.5517.403.30
HTSF-10.201.113.40230.00959.2011,953.8726.4723.782.690.810.972.8919.480.715.02
HTSF-20.183.852.90130.00599.508467.33122.54111.8810.660.520.915.3111.890.521.38
HTSF-40.632.707.90390.00719.406142.96156.91131.2325.680.701.022.964.690.651.33
HTSF-50.174.003.40100.00719.4019,009.9870.2266.883.341.000.917.7136.710.512.98
HTSF-100.300.334.00250.001618.657471.1717.7115.252.462.530.953.155.640.791.24
HTSF-110.302.346.001120.001258.9524,156.7880.1971.388.810.730.972.5820.090.735.71
HTSF-140.5615.908.15440.001678.6020,172.1695.4991.194.301.020.907.8625.760.431.70
HTSF-150.215.263.80740.001678.6010,957.7268.4866.831.651.270.977.0860.680.403.23
HTSF-160.501.195.30320.002398.008467.3367.8555.7012.150.710.962.993.250.690.82
HTSF-170.245.204.20790.002457.9515,440.42125.32117.537.790.861.023.7820.870.562.84
HTSF-180.210.413.75800.003297.2510,044.5730.7329.531.202.440.935.6831.180.462.52
HTSF-190.4115.735.80660.002038.3029,801.67157.10149.507.600.740.985.9526.620.472.20
HTSI-11.0010.8012.10150.002817.6521,085.30211.95172.0639.890.391.022.413.530.721.21
HTSI-20.384.235.20880.003656.9521,749.4197.9990.537.460.920.944.1817.390.622.29

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Figure 1. (A) The distribution of the basement in the North China Craton. (B) Regional geological map of the Qingyuan greenstone belt (after Fengjin Yu, (2005) [22]).
Figure 1. (A) The distribution of the basement in the North China Craton. (B) Regional geological map of the Qingyuan greenstone belt (after Fengjin Yu, (2005) [22]).
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Figure 2. (A) Hornblende-plagioclase gneiss; (B) sillimanite biotite plagioclase gneiss; (C) biotite plagioclase gneiss; (D) biotite plagioclase gneiss in the field; (E) garnet anthophyllite gneiss; (F) recrystallized garnet in garnet anthophyllite gneiss. (G) Stratigraphic column of Hongtoushan VMS deposit (after Fengjin Yu, (2005) [22]).
Figure 2. (A) Hornblende-plagioclase gneiss; (B) sillimanite biotite plagioclase gneiss; (C) biotite plagioclase gneiss; (D) biotite plagioclase gneiss in the field; (E) garnet anthophyllite gneiss; (F) recrystallized garnet in garnet anthophyllite gneiss. (G) Stratigraphic column of Hongtoushan VMS deposit (after Fengjin Yu, (2005) [22]).
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Figure 3. (A,B) Geological map and section map of No. 14 prospecting line in the Hongtoushan VMS deposit at the −167 m level (after Zhu, 2015 [25]). (C) Stereoscopic map of the ore body of the Hongtoushan VMS deposit (modified by Zhang, 2010 [5]).
Figure 3. (A,B) Geological map and section map of No. 14 prospecting line in the Hongtoushan VMS deposit at the −167 m level (after Zhu, 2015 [25]). (C) Stereoscopic map of the ore body of the Hongtoushan VMS deposit (modified by Zhang, 2010 [5]).
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Figure 4. (A,B) Cataclastic texture: the cracks of pyrite filled by plastic chalcopyrite; (C) porphyritic texture of pyrite; (D) different species of pyrite: cubic and granular in chalcopyrite surrounded by sphalerite; (E) chalcopyrite and pyrrhotite fill the fractures between pyrite and quartz; (F) the coexistence of Pyrite, chalcopyrite, sphalerite and pyrrhotite.(abbreviations: Py = pyrite; Po = pyrrhotite; Ccp = chalcopyrite; Sp = sphalerite).
Figure 4. (A,B) Cataclastic texture: the cracks of pyrite filled by plastic chalcopyrite; (C) porphyritic texture of pyrite; (D) different species of pyrite: cubic and granular in chalcopyrite surrounded by sphalerite; (E) chalcopyrite and pyrrhotite fill the fractures between pyrite and quartz; (F) the coexistence of Pyrite, chalcopyrite, sphalerite and pyrrhotite.(abbreviations: Py = pyrite; Po = pyrrhotite; Ccp = chalcopyrite; Sp = sphalerite).
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Figure 5. (A) CL images of the representative zircons; (B) Th and U concentration diagrams; (C) U-Pb zircon concordia diagrams for the HTS-1605-2 sample.
Figure 5. (A) CL images of the representative zircons; (B) Th and U concentration diagrams; (C) U-Pb zircon concordia diagrams for the HTS-1605-2 sample.
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Figure 6. (A) CL images of the representative zircons; (B) Th and U concentration diagrams; (C) U-Pb zircon concordia diagrams for sample HTS-1605-6.
Figure 6. (A) CL images of the representative zircons; (B) Th and U concentration diagrams; (C) U-Pb zircon concordia diagrams for sample HTS-1605-6.
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Figure 7. (A) CL images of the representative zircons; (B) Th and U concentration diagrams; (C) U-Pb zircon concordia diagrams for sample HTS-1605-9.
Figure 7. (A) CL images of the representative zircons; (B) Th and U concentration diagrams; (C) U-Pb zircon concordia diagrams for sample HTS-1605-9.
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Figure 8. (A) CL images of the representative zircons; (B) Th and U concentration diagrams; (C) U-Pb zircon concordia diagrams for sample HTS-1605-1.
Figure 8. (A) CL images of the representative zircons; (B) Th and U concentration diagrams; (C) U-Pb zircon concordia diagrams for sample HTS-1605-1.
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Figure 9. (A) CL images of the representative zircons; (B) Th and U concentration diagrams; (C) U-Pb zircon concordia diagrams for sample HTS-1605-3.
Figure 9. (A) CL images of the representative zircons; (B) Th and U concentration diagrams; (C) U-Pb zircon concordia diagrams for sample HTS-1605-3.
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Figure 10. (A) CL images of the representative zircons; (B) Th and U concentration diagrams; (C) U-Pb zircon concordia diagrams for sample HTS-1605-8.
Figure 10. (A) CL images of the representative zircons; (B) Th and U concentration diagrams; (C) U-Pb zircon concordia diagrams for sample HTS-1605-8.
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Figure 11. CCPI versus AI alteration box plot (Large et al. (2001) [39]).
Figure 11. CCPI versus AI alteration box plot (Large et al. (2001) [39]).
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Figure 12. (AH) Major (wt%) elements versus SiO   2 (wt%) diagrams and (IL) Zirconium (ppm) versus typical elements (ppm) diagrams of the ore-bearing host rocks in Hongtoushan.
Figure 12. (AH) Major (wt%) elements versus SiO   2 (wt%) diagrams and (IL) Zirconium (ppm) versus typical elements (ppm) diagrams of the ore-bearing host rocks in Hongtoushan.
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Figure 13. Primitive mantle-normalized trace element spider and chondrite-normalized REE pattern diagrams of rocks (AD) (normalizing values from Sun and McDonough [41]).
Figure 13. Primitive mantle-normalized trace element spider and chondrite-normalized REE pattern diagrams of rocks (AD) (normalizing values from Sun and McDonough [41]).
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Figure 14. (A) Diagram of Ga (ppm) versus Zr/TiO   2 for metamorphic rocks from the Hongtoushan VMS deposit. (B) Diagram of Nb/Y versus Zr/TiO   2 for metamorphic rocks from the Hongtoushan VMS deposit ((A,B) are both from Winchester and Floyd, 1997 [42]).
Figure 14. (A) Diagram of Ga (ppm) versus Zr/TiO   2 for metamorphic rocks from the Hongtoushan VMS deposit. (B) Diagram of Nb/Y versus Zr/TiO   2 for metamorphic rocks from the Hongtoushan VMS deposit ((A,B) are both from Winchester and Floyd, 1997 [42]).
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Figure 15. (A) Th/Yb versus Nb/Yb diagram of meta-host rocks from the Hongtoushan VMS deposit (modified from Hari et al. (2018) [53]). The N-MORB, E-MORB, and OIB (ocean island basalt) compositions are from Sun and McDonough (1989) [41]. The SCLM (sub-continental lithospheric mantle) composition is from McDonough (1990) [54]. Vectors CC and FC approximate the direction of crustal contamination and fractional crystallization, respectively. The dashed lines indicate the mantle array (Pearce 2008 [55]). (B) La/Sm versus Th/Nb diagram of Hongtoushan ore-bearing rocks (from Piercey et al. (2002) [56]).
Figure 15. (A) Th/Yb versus Nb/Yb diagram of meta-host rocks from the Hongtoushan VMS deposit (modified from Hari et al. (2018) [53]). The N-MORB, E-MORB, and OIB (ocean island basalt) compositions are from Sun and McDonough (1989) [41]. The SCLM (sub-continental lithospheric mantle) composition is from McDonough (1990) [54]. Vectors CC and FC approximate the direction of crustal contamination and fractional crystallization, respectively. The dashed lines indicate the mantle array (Pearce 2008 [55]). (B) La/Sm versus Th/Nb diagram of Hongtoushan ore-bearing rocks (from Piercey et al. (2002) [56]).
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Figure 16. (A) Nb/Yb versus Th/Yb (modified from Pearce (2008 [55]); (B) Zr/Y versus Nb/Y diagram modified by Condie et al. (2005) [57]. ARC = arc-related basalt; OPB = oceanic plateau basalt; OIB = oceanic island basalt; N-MORB = normal ocean ridge basalt; F = batch melting; SUB = subduction; orange arrow: a plume mixing array for early Archean non-arc basalts; blue arrow: a plume mixing array for late Archean non-arc basalts.
Figure 16. (A) Nb/Yb versus Th/Yb (modified from Pearce (2008 [55]); (B) Zr/Y versus Nb/Y diagram modified by Condie et al. (2005) [57]. ARC = arc-related basalt; OPB = oceanic plateau basalt; OIB = oceanic island basalt; N-MORB = normal ocean ridge basalt; F = batch melting; SUB = subduction; orange arrow: a plume mixing array for early Archean non-arc basalts; blue arrow: a plume mixing array for late Archean non-arc basalts.
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Table 1. Summary of Lu-Hf ages obtained in this study.
Table 1. Summary of Lu-Hf ages obtained in this study.
SampleLithologyMineralSize ( μ m)Hf(I) ε Hf(t)TDM1 (Ma)TDM2 (Ma)
HTS-1605-2Amphibole plagioclase gneisszircon50–120 (avg: 60–75)0.28128–0.281443.91–10.452453.51–2619.012411.13–2715.70
HTS-1605-6Amphibole plagioclase gneisszircon45–110 (avg: 70–80)0.28128–0.281394.30–8.452557.09–2687.692572.63–2776.15
HTS-1605-9Amphibole plagioclase gneisszircon70–150 (avg: 100–105)0.28131–0.281374.85–6.602568.22–2634.442607.11–2711.56
HTS-1605-1Biotite plagioclase gneisszircon60–90 (avg: 70–80)0.28130–0.281373.36–6.142558.37–2658.422615.79–2781.03
HTS-1605-3Biotite plagioclase gneisszircon40–110 (avg: 80–90)0.28126–0.281433.07–9.162489.97–2728.022469.98–2838.15
HTS-1605-8Biotite plagioclase gneisszircon50–80 (avg: 60–70)0.28136–0.281426.51–8.552498.84–2578.642494.38–2621.70
Note: Age (Ma) is the weighted mean   207 Pb/   206 Pb age; errors are δ ; n is the number of analyses. For the complete data, see Table A2.
Table 2. Major (wt%) and trace (rare earth) element composition and the relevant parameter ranges of the host rocks of the Hongtoushan VMS deposit.
Table 2. Major (wt%) and trace (rare earth) element composition and the relevant parameter ranges of the host rocks of the Hongtoushan VMS deposit.
Rock TypeAmphibole Plagioclase Gneiss
ValueAl   2 O   3 BaOCaOCr   2 O   3 Fe   2 O   3 TK   2 OMgOMnONa   2 OP   2 O   5 SiO   2 SrOTiO   2 LOITotal
Max16.670.0411.570.0613.212.977.420.223.710.3456.530.042.443.1999.90
Min14.250.023.02<0.018.750.343.170.102.270.0547.63<0.010.520.7299.60
Avg15.570.037.750.0311.211.144.980.163.210.1852.540.021.051.9699.82
ValueLaCePrNdSmEuGdTbDyHoErTmYbLuCo
Max28.3065.809.2239.408.812.668.651.287.061.453.690.503.210.4647.70
Min6.5014.501.898.001.940.581.990.352.060.411.150.181.060.1627.80
Avg12.0728.783.9917.334.201.174.190.683.980.832.320.342.210.3334.42
ValueNiCuZrSrYZnCsBaPbUVCrRbGaHf
Max130.0067.10267.00374.0036.40366.004.93277.0035.900.40245.00203.00105.2525.306.50
Min34.1010.9029.15118.509.7077.000.2059.301.700.13103.0020.003.5516.201.05
Avg65.8237.6593.81220.3321.38171.501.11162.228.930.24194.17110.1735.2919.332.52
ValueTaThNbPTiK Σ REE Σ LREE Σ HREE δ Eu δ Ce(La:Sm)   N (La:Yb)   N (Sm:Nd)   N (Gd:Yb)   N
Max1.303.7621.201490.0014,627.8024,654.86180.49154.1915.041.051.053.067.120.892.17
Min0.220.483.35220.003117.402822.4441.7833.817.510.620.961.141.510.681.16
Avg0.451.387.60800.006294.759421.9882.4267.5414.880.841.001.883.910.771.48
Rock TypeBiotite Plagioclase Gneiss
ValueAl   2 O   3 BaOCaOCr   2 O   3 Fe   2 O   3 TK   2 OMgOMnONa   2 OP   2 O   5 SiO   2 SrOTiO   2 LOITotal
Max16.460.114.840.046.763.594.790.115.850.2584.420.080.613.90100.10
Min6.940.010.77<0.011.640.740.330.021.930.0264.64<0.010.100.6399.03
Avg13.450.072.440.023.591.851.610.044.170.1170.440.040.311.6799.78
ValueLaCePrNdSmEuGdTbDyHoErTmYbLuCo
Max37.9078.709.8238.809.021.459.851.7510.552.366.850.996.580.9619.90
Min3.606.800.752.800.720.300.500.060.260.050.130.020.160.022.60
Avg20.3240.004.4816.513.170.752.820.462.540.531.470.221.430.238.49
ValueNiCuZrSrYZnCsBaPbUVCrRbGaHf
Max131.5080.40245.00723.0067.40585.007.322810.0034.303.3094.00196.00109.2520.907.00
Min2.102.9080.1547.301.3522.000.4878.703.200.169.0020.0014.108.562.20
Avg23.8921.36136.11306.6112.19103.431.79587.3910.910.7843.1466.5751.2815.943.66
ValueTaThNbPTiK Σ REE Σ LREE Σ HREE δ Eu δ Ce(La:Sm)   N (La:Yb)   N (Sm:Nd)   N (Gd:Yb)   N
Max1.0015.9012.101120.003656.9529,801.67211.95172.0639.892.531.027.8660.680.795.71
Min0.170.332.90100.00599.506142.9617.7115.251.200.390.902.413.250.400.82
Avg0.385.225.42500.001849.8915,351.4894.9385.239.691.050.964.6120.560.592.46
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You, X.; Wang, E.; Men, Y.; Fu, J.; Song, K.; Ma, S. The Zircon U-Pb Age, Hf Isotopes, and Lithogeochemistry of Ore-Bearing Rocks from the Archean Hongtoushan Volcanogenic Massive Sulfide Deposit in the North China Craton: Implications for Tectonic Setting. Minerals 2024, 14, 367. https://0-doi-org.brum.beds.ac.uk/10.3390/min14040367

AMA Style

You X, Wang E, Men Y, Fu J, Song K, Ma S. The Zircon U-Pb Age, Hf Isotopes, and Lithogeochemistry of Ore-Bearing Rocks from the Archean Hongtoushan Volcanogenic Massive Sulfide Deposit in the North China Craton: Implications for Tectonic Setting. Minerals. 2024; 14(4):367. https://0-doi-org.brum.beds.ac.uk/10.3390/min14040367

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You, Xinwei, Ende Wang, Yekai Men, Jianfei Fu, Kun Song, and Sishun Ma. 2024. "The Zircon U-Pb Age, Hf Isotopes, and Lithogeochemistry of Ore-Bearing Rocks from the Archean Hongtoushan Volcanogenic Massive Sulfide Deposit in the North China Craton: Implications for Tectonic Setting" Minerals 14, no. 4: 367. https://0-doi-org.brum.beds.ac.uk/10.3390/min14040367

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